CWNU 3992

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.15 0.75 0.0 0.28
C3
N_50
r_50
BA 23 4.8
Summary

CWNU 3992 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 177.811 -63.299 0.253 -5.544 0.734 –
           
UCC 177.92 -63.304 0.25 -5.524 0.722 -20.26
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3992 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.15, m-M=12.7, logA=7.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LISC 1273 72.0 177.92 -63.31 0.25 -5.54 0.72 – 0.33
CWWDL 873 4.0 177.89 -63.28 0.27 -5.67 0.73 – 0.08